Ministry of Science & Technology
Indigenously designed and developed ‘Made in India’ spectrograph, commissioned on Devasthal Optical Telescope, can locate faint light from distant celestial objects
Indian Scientists have indigenously designed and developed a low-cost optical spectrograph that can locate sources of faint light from distant quasars and galaxies in a very young universe, regions around supermassive black-holes around the galaxies, and cosmic explosions.
Such spectroscopes were so far imported from abroad involved high costs. The ‘Made in India’ optical spectrograph named as Aries-Devasthal Faint Object Spectrograph & Camera , indigenously designed and developed by Aryabhatta Research Institute of observational sciences , Nainital, an autonomous institute of Department of Science and Technology , Government of India, is about 2.5 times less costly compared to the imported ones and can locate sources of light with a photon-rate as low as about 1 photon per second.
The spectroscope, the largest of its kind among the existing astronomical spectrographs in the country, has been successfully commissioned on the 3.6-m Devasthal Optical Telescope , the largest in the country and in Asia, near Nainital Uttarakhand.
This instrument, a backbone of the 3.6-m DOT for observations of extremely faint celestial sources, uses a complex arrangement of several lenses made of special glasses, polished to better than 5-nanometer smoothness to produce sharp images of the celestial sky. Photons coming from distant celestial sources, collected by the telescope, are sorted into different colors by the spectrograph and are finally converted into electronic recordable signals using an in-house developed Charge-Coupled Device  camera cooled to an extremely low temperature of -120 0C. The total cost of this instrument is nearly Rs. 4 Crore.
Dr. Amitesh Omar, scientist at ARIES, led this project with a technical and scientific team, which together researched and developed various optical, mechanical, and electronics subsystems of the spectrograph and camera. The spectrograph is presently being used by astronomers from India and abroad to study distant quasars and galaxies in a very young universe, regions around supermassive black-holes around the galaxies, cosmic explosions like supernovae and highly energetic Gamma-ray bursts, young and massive stars, and faint dwarf galaxies.
“The indigenous efforts to build complex instruments like ADFOSC in India is an important step to become ‘Aatmanirbhar’ in the field of astronomy & astrophysics,” said Prof. Dipankar Banerjee, Director, ARIES.
Expertise from various national institutes, organizations, including the Indian Space Research Organization  and some micro-small-medium-enterprises, were involved to review and build parts of the instrument serving as an example of effective collaboration. With this expertise, ARIES now plans to commission more complex instruments such as spectro-polarimeter and high spectral resolution spectrograph on the 3.6-m Devasthal telescope in the near future.
This collage shows pictures of the 3.6-m Devasthal Optical Telescope , the ‘Made-in-India’ ARIES-Devasthal Faint Object Spectrograph & Camera , and an image of celestial source obtained from the telescope. The image of the Crab Nebulae shows the aftermath of a star explosion, which happened in the Milky-way galaxy in the year 1054. The color-coded optical spectrum obtained from ADFOSC shown here is of a recently dead massive star with spectral signatures of various elements such as Hydrogen, Iron, Sodium, Calcium, etc., once synthesized in its core and now being expelled out. This material becomes raw material to form new stars and planets in the future, thereby establishing the continuous cycle of birth and death of heavenly bodies.
[More details on the 3.6-m DOT and ADFOSC can be obtained from the URL:
https://www.aries.res.in/facilities/astronomical-telescopes/36m-telescope
https://www.currentscience.ac.in/Volumes/116/09/1472.pdf
For further details, Dr. Amitesh Omar, Scientist-F  can be contacted.]